CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves | Paper Citation Record

Observation 2cfb32f7-1c02-458d-9451-098028adbc8f · outbound

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

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Observation fe16cde3-e6a8-44e1-88b0-3f936158ddab · outbound

This paper cites To achieve this, we multiply the Gaussian realiza- tions from model 0 by a template that captures the spa- tial variations in foreground amplitudes.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves To achieve this, we multiply the Gaussian realiza- tions from model 0 by a template that captures the spa- tial variations in foreground amplitudes

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Observation cf7f2d41-fe78-4e0e-b0dd-f8e528b1ecde · outbound

This paper cites We first estimate foreground parameters and then reconstruct component maps (Sec.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves We first estimate foreground parameters and then reconstruct component maps (Sec

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Observation f8bfa6ee-5b3b-43b8-9568-23fd8a1c36a6 · outbound

This paper cites the most probable CMB lensing map.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves the most probable CMB lensing map

Reference 5

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Observation 87fd1479-172a-4adb-89f5-ed0eea004d12 · outbound

This paper cites Seljak and M.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Seljak and M

Reference 6

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Observation ba3f0db5-30bc-42be-aa60-fa6dafa1ab00 · outbound

This paper cites Most relevantly for our three cleaning methods, the low complexity suite (Model 3) is free of frequency decor- relation, while the medium complexity suite (Model.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Most relevantly for our three cleaning methods, the low complexity suite (Model 3) is free of frequency decor- relation, while the medium complexity suite (Model

Reference 7

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Observation 30a7738c-c76c-4acb-98a5-b7e7b8570a56 · outbound

This paper cites The high complexity suite (Model 5) incorporates a 3D model of the polarized dust emission, causing more complicated decorrelation effects.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves The high complexity suite (Model 5) incorporates a 3D model of the polarized dust emission, causing more complicated decorrelation effects

Reference 8

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Observation 46bd6f5f-5905-4524-b01c-a0226d3ffd88 · outbound

This paper cites Importantly, the simulations for Models 3, 4, and 5 all share the same noise realization, enabling a direct comparison of posterior results on equal footing.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Importantly, the simulations for Models 3, 4, and 5 all share the same noise realization, enabling a direct comparison of posterior results on equal footing

Reference 9

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Reference 10

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

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Observation 48aa1ca1-0ae4-45e7-a25c-08d14a470935 · outbound

This paper cites Sato, Mon.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Sato, Mon

Reference 12

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Observation 089510ab-958d-47cd-9965-62a1b74b0f19 · outbound

This paper cites Abazajian, G.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Abazajian, G

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Observation 800aebe5-13e6-4845-a27d-c9b31d7df8d0 · outbound

This paper cites Kamionkowski, A.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Kamionkowski, A

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Observation 7b2b54e1-9bd2-4de1-8617-0a3b7d2980ea · outbound

This paper cites Kamionkowski and E.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Kamionkowski and E

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Observation 1a89e569-3a7a-4592-a8ff-e6b08757edff · outbound

This paper cites Inflation: Theory and Observations.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Inflation: Theory and Observations

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Observation 3b980fda-23a1-4702-ba61-4fc63f23ea6b · outbound

This paper cites Snowmass2021 cosmic frontier: Cos- mic microwave background measurements white paper,.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Snowmass2021 cosmic frontier: Cos- mic microwave background measurements white paper,

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Observation 9074aad5-0ac1-425a-8402-4a3b4f246720 · outbound

This paper cites CLASS: The Cosmology Large Angular Scale Surveyor.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves CLASS: The Cosmology Large Angular Scale Surveyor

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Observation 50c4560b-885b-47b3-af23-a9b769d0367e · outbound

This paper cites A Constraint on Primordial $B$-Modes from the First Flight of the SPIDER Balloon-Borne Telescope.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves A Constraint on Primordial $B$-Modes from the First Flight of the SPIDER Balloon-Borne Telescope

Reference 21

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Observation 20788335-60ca-475f-afc9-eee36a40a690 · outbound

This paper cites The Simons Observatory: Science goals and forecasts.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves The Simons Observatory: Science goals and forecasts

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Observation 11d358f5-7b62-4bd2-b68f-e5f4fdc82d75 · outbound

This paper cites The Simons Observatory: pipeline comparison and validation for large-scale B-modes.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves The Simons Observatory: pipeline comparison and validation for large-scale B-modes

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This paper cites Cmb-s4 science book, first edition,.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Cmb-s4 science book, first edition,

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Observation 5cf2f779-ba42-45f8-a8ee-2fb15cbe7528 · outbound

This paper cites Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Allys, K

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Tristram, A

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This paper cites Bias on Tensor-to-Scalar Ratio Inference With Estimated Covariance Matrices.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Bias on Tensor-to-Scalar Ratio Inference With Estimated Covariance Matrices

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Campeti and E

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves de Belsunce, S

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Seljak and C

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Bezrukov and M

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Systematic errors in cosmic microwave background polarization measurements

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This paper cites Primordial B-mode Diagnostics and Self Calibrating the CMB Polarization.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Primordial B-mode Diagnostics and Self Calibrating the CMB Polarization

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This paper cites Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz

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Observation e4564d8b-3b86-478d-8364-c3f2f962e189 · outbound

This paper cites Verg` es, J.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Verg` es, J

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Knox and Y.-S

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Sparse component separation for accurate CMB map estimation

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Observation 4e91e14b-9aee-4179-9ea3-df4afe14de50 · outbound

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Akrami, M

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves The S-PASS view of polarized Galactic Synchrotron at 2.3 GHz as a contaminant to CMB observations

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves A method for subtracting foregrounds from multi-frequency CMB sky maps

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This paper cites Delabrouille, J.-F.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Delabrouille, J.-F

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Remazeilles, J

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Observation 9ed403ec-ee5b-4bfa-8db7-ab661a6aed9d · outbound

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Maino, A

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves SZ and CMB reconstruction using Generalized Morphological Component Analysis

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Component separation with flexible models. Application to the separation of astrophysical emissions

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Leloup, J

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Resolution: verified exact; doi, observed 2026-08-08T22:57:20.708107Z

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Pixel domain implementation of the Minimally Informed CMB MAp foreground Cleaning method

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Observation 0405d56d-653f-499e-acf6-7ec1efbc1e47 · outbound

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Stompor, S

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:57:22.381228Z

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Observation 57f9a5db-0e4a-4613-b4cc-f5f7b02d92e5 · outbound

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CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Errard, F

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Observation 951df036-65ad-4102-9f2f-a12571c22119 · outbound

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Observation 48ba06b2-481c-4ad2-84ae-c07574199026 · outbound

This paper cites Joint Bayesian component separation and CMB power spectrum estimation.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Joint Bayesian component separation and CMB power spectrum estimation

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Observation 70cbd40f-aebe-4b40-9eba-e8c714386caa · outbound

This paper cites de la Hoz, P.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves de la Hoz, P

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:57:22.355254Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 515f0bd6-122d-45d5-9b00-d047fd6e5ebe · outbound

This paper cites All-sky component separation in the presence of anisotropic noise and dust temperature variations.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves All-sky component separation in the presence of anisotropic noise and dust temperature variations

Reference 59

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:57:21.474422Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 4fc8503c-ab1a-4242-87cd-c26e83732ca0 · outbound

This paper cites Pseudo-$C_\ell$ estimators which do not mix E and B modes.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Pseudo-$C_\ell$ estimators which do not mix E and B modes

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.427606Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2e0325eb-5ebe-4134-85ff-ed3b8398ceb8 · outbound

This paper cites Bedini, D.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Bedini, D

Reference 61

Resolution: verified exact; arxiv_id_nonexistent, observed 2026-08-08T22:57:21.439876Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation d238628d-7314-46a6-b725-c7e68e917e6b · outbound

This paper cites Azzoni, D.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Azzoni, D

Reference 62

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:57:22.341831Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 07dd870a-b37b-45f5-ad07-0d1614a7b292 · outbound

This paper cites Multi-Clustering Needlet-ILC for CMB B-modes component separation.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Multi-Clustering Needlet-ILC for CMB B-modes component separation

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.398601Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bd06daaa-bdb8-465d-b597-a481dd0ecf32 · outbound

This paper cites Improved Galactic Foreground Removal for B-Modes Detection with Clustering Methods.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Improved Galactic Foreground Removal for B-Modes Detection with Clustering Methods

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:57:21.170150Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation b4852ceb-155c-4733-8c59-142d5478bf9c · outbound

This paper cites Hamimeche and A.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Hamimeche and A

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.408348Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 33720cab-c7ef-4a29-b0d2-9165425f5f83 · outbound

This paper cites BICEP2 / Keck Array x: Constraints on Primordial Gravitational Waves using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves BICEP2 / Keck Array x: Constraints on Primordial Gravitational Waves using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.413161Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 792101f3-9568-4138-9d0d-fe225a22f39b · outbound

This paper cites A Demonstration of Improved Constraints on Primordial Gravitational Waves with Delensing.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves A Demonstration of Improved Constraints on Primordial Gravitational Waves with Delensing

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.418218Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 805e0ccd-1572-4111-a51d-84b6f0da4e10 · outbound

This paper cites S2HAT: Scalable Spherical Harmonic Transform Library,.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves S2HAT: Scalable Spherical Harmonic Transform Library,

Reference 68

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:57:22.328439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 5f3e8873-1dde-403f-900d-5b0feeb34ae3 · outbound

This paper cites The Atacama Cosmology Telescope: High-resolution component-separated maps across one-third of the sky.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves The Atacama Cosmology Telescope: High-resolution component-separated maps across one-third of the sky

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.471363Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5a8a094-1234-436e-a2ae-2becc5f23718 · outbound

This paper cites Polarized CMB power spectrum estimation using the pure pseudo-cross-spectrum approach.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Polarized CMB power spectrum estimation using the pure pseudo-cross-spectrum approach

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.432534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ef760d76-f3c3-44b4-b6c9-24408580b17e · outbound

This paper cites an unresolved cited work.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

Reference 71

Resolution: unresolved; raw_fallback, observed 2026-08-08T22:57:22.314499Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation e19e336b-95e4-429d-80a4-28d2449e3954 · outbound

This paper cites an unresolved cited work.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

Reference 73

Resolution: unresolved; raw_fallback, observed 2026-08-08T22:57:22.300848Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation e3e86fe0-2540-443d-9f52-ce4a9abf7ff9 · outbound

This paper cites Impact of calibration errors on CMB component separation using FastICA and ILC.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Impact of calibration errors on CMB component separation using FastICA and ILC

Reference 74

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:57:21.091237Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation fb38911c-870b-443b-b050-217e64467f83 · outbound

This paper cites A unified pseudo-$C_\ell$ framework.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves A unified pseudo-$C_\ell$ framework

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.456180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 67c6ba8a-3462-44f0-8000-618ec6dae374 · outbound

This paper cites Validating a main beam treatment of parametric, pixel-based component separation in the context of CMB observations.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Validating a main beam treatment of parametric, pixel-based component separation in the context of CMB observations

Reference 76

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:57:21.054604Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation d18373e2-5bfe-4861-8591-e1891ad7acf3 · outbound

This paper cites an unresolved cited work.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

Reference 77

Resolution: verified exact; doi, observed 2026-08-08T22:57:20.668534Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation b7cac1e0-2308-43f9-8efc-b1c3df21c2b9 · outbound

This paper cites A 3D model for CO molecular line emission as a potential CMB polarization contaminant.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves A 3D model for CO molecular line emission as a potential CMB polarization contaminant

Reference 78

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:57:20.980520Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 29d09f5e-5456-41f3-b715-4b943449934b · outbound

This paper cites Basak and J.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Basak and J

Reference 79

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:57:22.286727Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation ab9adcbd-541f-4dec-b834-3048b47ea323 · outbound

This paper cites an unresolved cited work.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

Reference 80

Resolution: malformed identifier; no resolver link, observed 2026-08-08T22:57:20.480900Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 26b26b35-d296-4528-8390-38f8c733cc19 · outbound

This paper cites an unresolved cited work.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

Reference 81

Resolution: unresolved; raw_fallback, observed 2026-08-08T22:57:22.272952Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 7d35a069-1581-47e5-8afd-1db99cc681aa · outbound

This paper cites Aghanim, Y.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Aghanim, Y

Reference 82

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:57:22.259008Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 8db70e3f-134d-47c4-b534-f4262d2c40cd · outbound

This paper cites an unresolved cited work.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

Reference 83

Resolution: unresolved; raw_fallback, observed 2026-08-08T22:57:22.244904Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 2501a515-0ba7-44bc-be39-d1902d79f2a5 · outbound

This paper cites Statistical simulations of the dust foreground to CMB polarization.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Statistical simulations of the dust foreground to CMB polarization

Reference 84

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:57:21.017310Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation c902417b-80b0-43c1-8333-ea1bf936cff3 · outbound

This paper cites Planck intermediate results. L. Evidence for spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB $B$-mode analysis.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Planck intermediate results. L. Evidence for spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB $B$-mode analysis

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.503351Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f5968dc3-661d-4313-849e-41689bf38408 · outbound

This paper cites Thorne, J.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Thorne, J

Reference 86

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:57:22.229989Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation b2a3b2b1-0606-427b-99ae-fe3ee0e8c4fd · outbound

This paper cites LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.553272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fc3b3d8e-1a38-47f8-8282-bd4f13a44b0b · outbound

This paper cites Mart ´ ınez-Solaeche, A.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Mart ´ ınez-Solaeche, A

Reference 88

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:57:22.214667Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 6829167c-808d-4ac0-98c5-c79179b70d19 · outbound

This paper cites Synchrotron Spectral Curvature from 22 MHz to 23 GHz.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Synchrotron Spectral Curvature from 22 MHz to 23 GHz

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.521527Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5464597d-4321-4d1a-b6d7-37fc6a13eb33 · outbound

This paper cites Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER

Reference 90

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:57:20.943977Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 1c9b7e0e-6343-4459-80cb-354e06e17b99 · outbound

This paper cites an unresolved cited work.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

Reference 91

Resolution: unresolved; raw_fallback, observed 2026-08-08T22:57:22.200718Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation f2aa8fa7-0cfb-4d8a-b344-e63d9204ba53 · outbound

This paper cites an unresolved cited work.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

Reference 92

Resolution: verified exact; doi, observed 2026-08-08T22:57:20.653474Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation fb9fd354-d1c5-459f-a75d-e5982267cd02 · outbound

This paper cites Maximum a posteriori CMB lensing reconstruction.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Maximum a posteriori CMB lensing reconstruction

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.539729Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0452121b-070d-4b5a-9531-83fa0c7611eb · outbound

This paper cites Millea, E.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Millea, E

Reference 94

Resolution: verified exact; doi, observed 2026-08-08T22:57:20.637875Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 0c864135-b1bc-46c0-8612-8206a21ab9c7 · outbound

This paper cites LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMB.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMB

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.548751Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 21591f5f-8854-42b5-9bfe-ea47f02f043c · outbound

This paper cites Characterizing bias on large scale CMB $B$-modes after galactic foregrounds cleaning.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Characterizing bias on large scale CMB $B$-modes after galactic foregrounds cleaning

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.594826Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ab7cb289-fd21-437b-8c8b-d103cebbe062 · outbound

This paper cites CMB-S4: Iterative Internal Delensing and $r$ Constraints.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves CMB-S4: Iterative Internal Delensing and $r$ Constraints

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.557830Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f81be903-506c-46f1-8fd5-7bf60c51145d · outbound

This paper cites Cosmic Microwave Background Delensing Revisited: Residual Biases and a Simple Fix.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Cosmic Microwave Background Delensing Revisited: Residual Biases and a Simple Fix

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.563005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation de09137b-003c-4341-a9ec-bb0531d797d3 · outbound

This paper cites an unresolved cited work.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Unresolved cited work

Reference 99

Resolution: unresolved; raw_fallback, observed 2026-08-08T22:57:22.186189Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 71f1daec-20f7-4854-831f-4e13c12cf071 · outbound

This paper cites The Atacama Cosmology Telescope: Delensed Power Spectra and Parameters.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves The Atacama Cosmology Telescope: Delensed Power Spectra and Parameters

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.572551Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1aed9c61-d62e-4f90-b926-8ac58ec27a09 · outbound

This paper cites Limitations of CMB B-mode template delensing.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Limitations of CMB B-mode template delensing

Reference 101

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:57:20.837105Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation c647f30b-12f8-408e-824b-cc4631de8593 · outbound

This paper cites CAMB: Code for Anisotropies in the Microwave Background,.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves CAMB: Code for Anisotropies in the Microwave Background,

Reference 102

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:57:22.171972Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 94ee5a58-4c1c-4d84-b370-02c7fcb47712 · outbound

This paper cites Why your model parameter confidences might be too optimistic -- unbiased estimation of the inverse covariance matrix.

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves Why your model parameter confidences might be too optimistic -- unbiased estimation of the inverse covariance matrix

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-08T22:57:20.585788Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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